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1. The Infrared Auroral Footprint Tracks of Io, Europa and Ganymede at Jupiter Observed by Juno‐JIRAM

3. Source of Radio Emissions Induced by the Galilean Moons Io, Europa and Ganymede: In Situ Measurements by Juno

5. Variability of the Auroral Footprint of Io Detected by Juno‐JIRAM and Modeling of the Io Plasma Torus

6. Juno's Multi‐Instruments Observations During the Flybys of Auroral Bright Spots in Jupiter's Polar Aurorae

8. Evidence for Non‐Monotonic and Broadband Electron Distributions in the Europa Footprint Tail Revealed by Juno In Situ Measurements

9. Poynting Fluxes, Field‐Aligned Current Densities, and the Efficiency of the Io‐Jupiter Electrodynamic Interaction

10. The Io, Europa, and Ganymede Auroral Footprints at Jupiter in the Ultraviolet: Positions and Equatorial Lead Angles

11. Supplemental Tables S1-S12 from Genomic and Transcriptomic Analysis of Relapsed and Refractory Childhood Solid Tumors Reveals a Diverse Molecular Landscape and Mechanisms of Immune Evasion

12. Figure S6 from Genomic and Transcriptomic Analysis of Relapsed and Refractory Childhood Solid Tumors Reveals a Diverse Molecular Landscape and Mechanisms of Immune Evasion

13. Figure S2 from Genomic and Transcriptomic Analysis of Relapsed and Refractory Childhood Solid Tumors Reveals a Diverse Molecular Landscape and Mechanisms of Immune Evasion

14. Figure S1 from Genomic and Transcriptomic Analysis of Relapsed and Refractory Childhood Solid Tumors Reveals a Diverse Molecular Landscape and Mechanisms of Immune Evasion

15. Data from Genomic and Transcriptomic Analysis of Relapsed and Refractory Childhood Solid Tumors Reveals a Diverse Molecular Landscape and Mechanisms of Immune Evasion

16. Data from Genomic and Transcriptomic Analysis of Relapsed and Refractory Childhood Solid Tumors Reveals a Diverse Molecular Landscape and Mechanisms of Immune Evasion

17. Figure S4 from Genomic and Transcriptomic Analysis of Relapsed and Refractory Childhood Solid Tumors Reveals a Diverse Molecular Landscape and Mechanisms of Immune Evasion

18. Figure S5 from Genomic and Transcriptomic Analysis of Relapsed and Refractory Childhood Solid Tumors Reveals a Diverse Molecular Landscape and Mechanisms of Immune Evasion

19. Figure S3 from Genomic and Transcriptomic Analysis of Relapsed and Refractory Childhood Solid Tumors Reveals a Diverse Molecular Landscape and Mechanisms of Immune Evasion

20. Energetic proton acceleration by EMIC waves in Io’s footprint tail

22. UVS Observations of Ganymede's Aurora During Juno Orbits 34 and 35

23. Ganymede's UV Reflectance From Juno‐UVS Data

27. Jupiter's Low‐Altitude Auroral Zones: Fields, Particles, Plasma Waves, and Density Depletions

29. Loss of Energetic Ions Comprising the Ring Current Populations of Jupiter's Middle and Inner Magnetosphere

30. A Comprehensive Set of Juno In Situ and Remote Sensing Observations of the Ganymede Auroral Footprint

31. Genomic and Transcriptomic Analysis of Relapsed and Refractory Childhood Solid Tumors Reveals a Diverse Molecular Landscape and Mechanisms of Immune Evasion

32. Simultaneous UV Images and High‐Latitude Particle and Field Measurements During an Auroral Dawn Storm at Jupiter

33. Immuno-transcriptomic profiling of extracranial pediatric solid malignancies

38. Magnetospheric Studies: A requirement for addressing interdisciplinary mysteries in the Ice Giant systems

39. Detection and Characterization of Circular Expanding UV‐Emissions Observed in Jupiter's Polar Auroral Regions

40. First direct measurement of auroral and equatorial jets in the stratosphere of Jupiter

41. Are Dawn Storms Jupiter's Auroral Substorms?

42. Morphology of Jupiter's Polar Auroral Bright Spot Emissions via Juno‐UVS Observations

44. Energetic Proton Acceleration Associated With Io's Footprint Tail

46. Wave‐Particle Interactions Associated With Io's Auroral Footprint: Evidence of Alfvén, Ion Cyclotron, and Whistler Modes

48. A New Framework to Explain Changes in Io's Footprint Tail Electron Fluxes

49. First Report of Electron Measurements During a Europa Footprint Tail Crossing by Juno

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